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Dwarf elliptical galaxies as probes of galaxy formation and evolution
Marina Trevisan
Reinaldo de Carvalho, Fabricio Ferrari, Ignacio Ferreras, Francesco la Barbera, Ignacio de la Rosa
24 April 2013
Galaxy Formation and Evolution
● Galaxy evolution/formation scenario must be able to predict and describe the properties of galaxies in all mass ranges.
● Different processes acting in galaxies with different masses:
– SN/AGN feedback;
– IMF;
– Environment...
● Dificuldade na classificação
M (M☉)
5 ∙ 10111 ∙ 10111 ∙ 10101 ∙ 1095 ∙ 108
Elliptical Galaxies
dwarfs
Galaxy Zoo Project
Visual Classification
Parameter Space
Elliptical M > 3 ∙ 1010 M☉
Elliptical M > 3 ∙ 1010 M☉
Elliptical M < 1 ∙ 1010 M☉
Elliptical M < 1 ∙ 1010 M☉
Spiral M < 1 ∙ 1010 M☉Spiral M < 1 ∙ 1010 M☉
Asymmetry
Sersic index
Concentration
Asymmetry
Concentration
Sersic index
● Dwarf sample:
– Stellar population analysis Star formation history, →chemical enrichment
Formation and Evolution of Dwarf ETGs
de la Rosa et al. 2011
Trevisan et al. 2012
Mass Assembly
Trevisan et al. 2012
Chemical Enrichment
● Dwarf sample:
– Stellar population analysis Star formation history, →chemical enrichment
● Different environments
Formation and Evolution of Dwarf ETGs
Formation and Evolution of Dwarf ETGs
● Dwarf sample:
– Stellar population analysis Star formation history, →chemical enrichment
● Different environments
– Explore stellar population properties in the outer regions
→ Web-Starlight
→SSP models with variable chemical abundances
Correlations between galaxy properties and evolutionary
stage of groups
Correlation between
σ and IMF slope
Radial gradients with VLT data
2013
2012
Thank you!